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  Influence of Internal Structure on the Motion of Test Bodies in Extreme Mass Ratio Situations

Steinhoff, J., & Puetzfeld, D. (2015). Influence of Internal Structure on the Motion of Test Bodies in Extreme Mass Ratio Situations. In K. Rosquist, R. T. Jantzen, & R. Ruffini (Eds.), Proceedings of the MG13 Meeting on General Relativity (pp. 978-980). World Scientific.

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Item Permalink: http://hdl.handle.net/11858/00-001M-0000-0025-039D-C Version Permalink: http://hdl.handle.net/11858/00-001M-0000-0025-039E-A
Genre: Conference Paper

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 Creators:
Steinhoff, Jan1, Author              
Puetzfeld, Dirk, Author
Affiliations:
1Astrophysical and Cosmological Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society, escidoc:1933290              

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 Abstract: We present some recent results on the motion of test bodies with internal structure in General Relativity. On the basis of a multipolar approximation scheme, we study the motion of extended test bodies endowed with an explicit model for the quadrupole. The model is inspired by effective actions recently proposed in the context of the post-Newtonian approximation, including spin-squared and tidal contributions. In the equatorial plane of the Kerr geometry, the motion can be characterized by an effective potential of the binding energy. We compare our findings to recent results for the conservative part of the self-force in astrophysically realistic situations.

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 Dates: 2015
 Publication Status: Published in print
 Pages: -
 Publishing info: -
 Table of Contents: -
 Rev. Method: -
 Identifiers: DOI: 10.1142/9789814623995_0060
 Degree: -

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Title: The Thirteenth Marcel Grossmann Meeting
Place of Event: Stockholm University, Sweden
Start-/End Date: 2012-07-01 - 2012-07-07

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Title: Proceedings of the MG13 Meeting on General Relativity
Source Genre: Proceedings
 Creator(s):
Rosquist , Kjell , Editor
Jantzen , Robert T., Editor
Ruffini , Remo , Editor
Affiliations:
-
Publ. Info: World Scientific
Pages: - Volume / Issue: - Sequence Number: - Start / End Page: 978 - 980 Identifier: -